Gravitational wave denoising of binary black hole mergers with deep learning

Gravitational wave detection requires an in-depth understanding of the physical properties of gravitational wave signals, and the noise from which they are extracted. Understanding the statistical properties of noise is a complex endeavor, particularly in realistic detection scenarios. In this artic...

Full description

Bibliographic Details
Main Authors: Wei Wei, E.A. Huerta
Format: Article
Language:English
Published: Elsevier 2020-01-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269319308032
id doaj-b7f29c2cda0c49088bfeedbb3171a093
record_format Article
spelling doaj-b7f29c2cda0c49088bfeedbb3171a0932020-11-25T01:29:51ZengElsevierPhysics Letters B0370-26932020-01-01800Gravitational wave denoising of binary black hole mergers with deep learningWei Wei0E.A. Huerta1NCSA, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA; Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA; Corresponding author.NCSA, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA; Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USAGravitational wave detection requires an in-depth understanding of the physical properties of gravitational wave signals, and the noise from which they are extracted. Understanding the statistical properties of noise is a complex endeavor, particularly in realistic detection scenarios. In this article we demonstrate that deep learning can handle the non-Gaussian and non-stationary nature of gravitational wave data, and showcase its application to denoise the gravitational wave signals generated by the binary black hole mergers GW150914, GW170104, GW170608 and GW170814 from advanced LIGO noise. To exhibit the accuracy of this methodology, we compute the overlap between the time-series signals produced by our denoising algorithm, and the numerical relativity templates that are expected to describe these gravitational wave sources, finding overlaps O≳0.99. We also show that our deep learning algorithm is capable of removing noise anomalies from numerical relativity signals that we inject in real advanced LIGO data. We discuss the implications of these results for the characterization of gravitational wave signals. Keywords: Gravitational waves, Deep learning, Denoising, Black holes, LIGOhttp://www.sciencedirect.com/science/article/pii/S0370269319308032
collection DOAJ
language English
format Article
sources DOAJ
author Wei Wei
E.A. Huerta
spellingShingle Wei Wei
E.A. Huerta
Gravitational wave denoising of binary black hole mergers with deep learning
Physics Letters B
author_facet Wei Wei
E.A. Huerta
author_sort Wei Wei
title Gravitational wave denoising of binary black hole mergers with deep learning
title_short Gravitational wave denoising of binary black hole mergers with deep learning
title_full Gravitational wave denoising of binary black hole mergers with deep learning
title_fullStr Gravitational wave denoising of binary black hole mergers with deep learning
title_full_unstemmed Gravitational wave denoising of binary black hole mergers with deep learning
title_sort gravitational wave denoising of binary black hole mergers with deep learning
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2020-01-01
description Gravitational wave detection requires an in-depth understanding of the physical properties of gravitational wave signals, and the noise from which they are extracted. Understanding the statistical properties of noise is a complex endeavor, particularly in realistic detection scenarios. In this article we demonstrate that deep learning can handle the non-Gaussian and non-stationary nature of gravitational wave data, and showcase its application to denoise the gravitational wave signals generated by the binary black hole mergers GW150914, GW170104, GW170608 and GW170814 from advanced LIGO noise. To exhibit the accuracy of this methodology, we compute the overlap between the time-series signals produced by our denoising algorithm, and the numerical relativity templates that are expected to describe these gravitational wave sources, finding overlaps O≳0.99. We also show that our deep learning algorithm is capable of removing noise anomalies from numerical relativity signals that we inject in real advanced LIGO data. We discuss the implications of these results for the characterization of gravitational wave signals. Keywords: Gravitational waves, Deep learning, Denoising, Black holes, LIGO
url http://www.sciencedirect.com/science/article/pii/S0370269319308032
work_keys_str_mv AT weiwei gravitationalwavedenoisingofbinaryblackholemergerswithdeeplearning
AT eahuerta gravitationalwavedenoisingofbinaryblackholemergerswithdeeplearning
_version_ 1725094329296355328